The semiclassical limit from the Pauli-Poisswell/Darwin to the Euler-Poisswell/Darwin system by WKB methods
Norbert J. Mauser, Jakob M\"oller, Changhe Yang

TL;DR
This paper derives the semiclassical limit of semi-relativistic Pauli equations to classical Euler-Poisswell/Darwin systems using WKB methods, connecting quantum spin models to classical plasma dynamics.
Contribution
It establishes the rigorous semiclassical limit from Pauli-Poisswell/Darwin equations to Euler-Poisswell/Darwin systems, including convergence results and well-posedness analysis.
Findings
Proved local in time semiclassical limit $ abla ightarrow 0$ to Euler-Poisswell/Darwin equations.
Established weak convergence of Wigner transforms to Vlasov-type equations.
Proved local well-posedness and blow-up criteria for the Euler-Poisswell/Darwin equations.
Abstract
The self-consistent Pauli-Poisswell and Pauli-Darwin equations for 2-spinors are (where denotes the speed of light) semi-relativistic approximations of the Dirac-Maxwell equation for 4-spinors coupled to the self-consistent electromagnetic fields generated by the charge and current densities of a fast moving electric charge. They consist of a vector-valued magnetic Schr\"odinger equation with the Stern-Gerlach term which couples spin and magnetic field, coupled to 1+3 Poisson equations as the magnetostatic approximation of Maxwell's equations. The Pauli-Poisswell and Pauli-Dariwn euqations are models keeping both relativistic effects magnetism and spin, both of which are absent in the non-relativistic Schr\"odinger-Poisson equation and inconsistent in the magnetic Schr\"odinger-Maxwell equation. We prove the local in time semiclassical limit $\hbar \rightarrow…
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Taxonomy
TopicsSpectral Theory in Mathematical Physics · Quantum Mechanics and Non-Hermitian Physics · Advanced Mathematical Physics Problems
